Meridional polar slices of gas phase element abundance log ₁₀ε_i = n_i/n_{⟨ H ⟩} (ratio i to hydrogen abundance) of top: Ti (blue), second row: O (red), third row: Si (purple) and fourth row: Mg (orange/brown) at θ = 0° (left) and θ = 45° (right), respectively. For reference, solar metallicity of the elements from Asplund et al. (2009) are, Ti: −7.05, O: −3.31, Si: −4.49, Mg: −4.40. Lighter coloured regions indicate a depletion of elements due to the cloud formation processes. Darker coloured regions indicate a local element abundance closer to the initial solar values. Outer circular values denote longitude at intervals of φ = 45° from the sub-stellar point (φ = 0°). Radial values indicate log ₁₀p_gas isobars from 0.1 mbar−100 bar. The globe is irradiated from the direction of the colour bars. Note: the size of the annulus is not scaled to planetary radius.